collaborators

8 papers

astro-ph.SR2026

Correlations with Magnetic Activity in the Solar Near-Surface Shear Layer. II. Radial Shear

M. Cristina Rabello Soares, Sarbani Basu, Richard S. Bogart +1

Using Helioseismic and Magnetic Imager ring-diagram measurements and building on the rotation-rate inferences presented in Paper I for depths of 1-17 Mm, we examine the propert…

astro-ph.SR2026

Correlations with Magnetic Activity in the Solar Near-Surface Shear Layer. I. Rotation

M. Cristina Rabello Soares, Sarbani Basu, Richard S. Bogart

We used data from the Helioseismic and Magnetic Imager to determine the rotation rate of the near-surface shear layer and its time variation. We applied the ring-diagram analysis t…

astro-ph.SR2026

Sub-surface structural changes associated with successive 11-yr solar activity cycles have been progressively more confined near the surface: new helioseismic results on Cycles 22 -- 25 from BiSON

William J. Chaplin, Sarbani Basu, Rachel Howe +3

We use Sun-as-a-star helioseismology data, collected by the Birmingham Solar-Oscillations Network (BiSON), to examine the relationship between the solar-cycle-induced frequency shi…

astro-ph.SR2026

Latitude-Dependent Time Variations of the Solar Tachocline

Sarbani Basu, Sylvain G. Korzennik, Sushanta C. Tripathy

We have examined how the characteristics of the tachocline -- i.e., the change in rotation rate , or the "jump", the position of the midpoint of the tachocline, , and th…

astro-ph.SR2026

The seismic diversity of four successive solar cycle minima as observed by the Birmingham Solar-Oscillations Network (BiSON)

Sarbani Basu, William J. Chaplin, Rachel Howe +3

We have used data collected by the Birmingham Solar-Oscillations Network (BiSON) to perform a helioseismic diagnosis of changes to the Sun's internal structure between four success…

astro-ph.SR2026

Constraints on sunspot group lifetimes from far-side Sun-as-a-star helioseismology with BiSON

William J. Chaplin, Rachel Howe, Sarbani Basu +5

Frequencies of low-degree solar p modes are sensitive to activity over the entire Sun, including the unobservable far-side hemisphere. When frequency shifts extracted from week-lon…